dot
Detailansicht
Katalogkarte GBA
Katalogkarte ISBD
Suche präzisieren
Drucken
Download RIS
Hier klicken, um den Treffer aus der Auswahl zu entfernen
Titel An Energy Backscatter Model For The Shallow Water Equations On The Sphere
VerfasserIn James Kent, Christiane Jablonowski, John Thuburn, Nigel Wood
Konferenz EGU General Assembly 2014
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 16 (2014)
Datensatznummer 250088909
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2014-3085.pdf
 
Zusammenfassung
Many atmospheric dynamical cores conserve total energy through the use of energy fixers. These energy fixers replace dissipated kinetic energy with temperature. A more accurate method could conserve energy by adding back both temperature and kinetic energy, with the kinetic energy added at the large scales to represent the inverse energy cascade (backscatter). We focus on the shallow water equations on the sphere which are a common building block of dynamical cores. We present an energy backscatter model that replaces dissipated energy with both kinetic and potential energy. We apply the backscatter model to two shallow water schemes, both based on semi-Lagrangian numerics, and perform a series of tests using well known shallow water equation test cases. The results show that the application of the backscatter model successfully conserves total energy without affecting the conservation of other quantities (such as mass).